|2004 Denver Annual Meeting (November 7–10, 2004)|
|Paper No. 110-13|
|Presentation Time: 5:05 PM-5:20 PM|
THE HORSESHOE-SHAPED RIM OF WETUMPKA MARINE IMPACT CRATER -- FROM OBLIQUE IMPACT OR HETEROGENEITY IN THE RIM?
KING, David T. Jr, Dept. Geology, Auburn Univ, Auburn, AL 36849, firstname.lastname@example.org, PETRUNY, Lucille W., Astra-Terra Rsch, Auburn, AL 36831-3323, and NEATHERY, Thornton L., 1212-H Veterans Memorial Parkway, Tuscaloosa, AL 35404|
Wetumpka impact structure is a Late Cretaceous impact feature of the inner Gulf coastal plain of Alabama. The shape of Wetumpka's rim is similar to a horseshoe (encompassing ~ 270 degrees of arc). The southwestern quadrant is topographically open (i.e., the land is rather flat) and free of crystalline rock exposures that characterize the balance of the rim. In view of experimental results with oblique impactors, Wetumpka would appear to be a clear-cut example of an low-angle impact where the trajectory was southwest (causing rim blow-out on the southwest). However, the underlying geology of the area and the marine-impact origin of this structure point to a different scenario for development of the horseshoe shape. The target was composed of a water layer, underlain by semi-consolidated Upper Cretaceous sedimentary units (~ 100 m thick) lying on hard crystalline rock. Wetumpka impact occurred ~ 25 km offshore in water ~ 30 to 100 m deep. Final rim height exceeded water depth, and a continuous (360 degree) rim likely persisted for some time after impact enabling a short-lived terrestrial ecosystem to form within. Evidence for this history was acquired during core drilling at crater center, which revealed a paleosol layer at ~ 67 m depth. This paleosol separates > 100 m of lower fall-back and wash-back breccias from overlying displaced sedimentary materials. Based on their structures and textures, these upper displaced materials appear to be the deposits of a late-stage, catastrophic rim collapse that washed sediment-water slurries and entrained sedimentary megablocks onto the crater floor. Local bedrock dip (~ 15m/km) to the southwest explains target sedimentary cover that was thicker on the southwestern quadrant of the impact structure than elsewhere. This effect likely resulted in the southwestern rim being composed mainly of Upper Cretaceous sedimentary target, whereas the balance of the rim was formed mainly of hard, crystalline target (Piedmont bedrock). This heterogeneity of rim material seems more likely to account for the rim's subsequent failure and resulting catastrophic flood emplacement of the crater-floor sedimentary cover that obliquity of the impactor. This instance shows how difficult it is to assess obliquity of impact based solely upon surface morphology of an impact structure.
2004 Denver Annual Meeting (November 7–10, 2004)
General Information for this Meeting
|Session No. 110|
Impact Geology II
Colorado Convention Center: 111/113
1:30 PM-5:30 PM, Monday, 8 November 2004
Geological Society of America Abstracts with Programs, Vol. 36, No. 5, p. 266
© Copyright 2004 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.